PHYSICAL PROPERTIES OF EMISSION-LINE GALAXIES AT z ~ 2 FROM NEAR-INFRARED SPECTROSCOPY WITH MAGELLAN FIRE (2014)
Attributed to:
Star formation and mass assembly at the highest redshifts
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1088/0004-637x/785/2/153
Publication URI: http://dx.doi.org/10.1088/0004-637x/785/2/153
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 2
ISSN: 0004-637X